@article{furnstahl_new_2013,
abstract = {We give an overview of recent results for the nuclear equation of state and properties of neutron stars based on microscopic two- and three-nucleon interactions derived within chiral effective field theory (EFT). It is demonstrated that the application of Renormalization Group (RG) transformations allows efficient, controlled and simplified calculations of nuclear matter. {\textcopyright} 2013 AIP Publishing LLC.},
archivePrefix = {arXiv},
arxivId = {1208.4297},
author = {Hebeler, Kai},
doi = {10.1063/1.4826857},
eprint = {1208.4297},
isbn = {9780735411883},
issn = {0094243X},
journal = {AIP Conference Proceedings},
keywords = {Neutron stars,Nuclear equation of state,Renormalization Group,Three-nucleon forces},
number = {12},
pages = {626--630},
title = {{New applications of renormalization group methods to nuclear matter}},
url = {http://stacks.iop.org/0034-4885/76/i=12/a=126301},
volume = {1560},
year = {2013}
}

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